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The Minkowski vacuum model with Lambda = 0: field law, free-fall kinematics and clock readings
Conditional model deduction inside the classical gravitational framework with the field law in its direct-equation presentation: the flat model spacetime R^4 with the Minkowski metric, zero cosmological parameter and the vacuum stress-energy content T=0 is a model of the framework satisfying the adopted field law, and its ideal free-fall worldlines and ideal-clock readings are the straight timelike lines and their proper times. Clause (d) additionally compares this model with explicitly constructed flat quotient and non-flat vacuum models to establish that the same field law does not uniquely select the R^4 Minkowski geometry. The free-fall and clock conclusions (b)-(c) concern only the stated Minkowski model. Excludes: any claim that these vacua are realized in nature, any empirical comparison (no observations, apparatus, calibration or uncertainty are used), non-vacuum matter, nonzero Lambda, distributional sources and quantum effects. All conclusions are conditional on the adopted postulates.
Statement
Adopt the postulates Adopted spacetime model and classical domain of the gravitational framework, Adopted matter-content assumptions: fields, equations, stress-energy and energy conditions, Adopted Einstein field equation in the direct-equation presentation and Adopted clock, free-fall and light-ray assumptions of the classical gravitational framework of the classical gravitational framework, with the field law in its direct-equation presentation. Let be the flat model of The flat model spacetime: the Minkowski metric on R^4 and its inertial chart with inertial chart , let and let the model's stress-energy tensor be the vacuum prescription
Then all statements below are conditional deductions inside the model so specified; they assert nothing about nature.
(a) The flat vacuum model. satisfies the spacetime postulate, is a smooth symmetric stress-energy tensor field on the matter domain in the sense of Stress-energy tensor field of a model, the prescription is admissible, and the adopted field law holds identically on ; in the notation of Consistency conditions of the adopted field law: conservation, trace, parameter variation and the energy conditions of a perfect fluid clause (d) this is its flat vacuum solution, here read as a model of the framework.
(b) Free fall and clocks. Let and let be future timelike with . In the inertial chart write and with and . Then the physical worldline of an ideal freely falling massive test body released at with four-velocity , with proper-time origin at release, is a restriction to its actual proper-time interval of the unique maximal mathematical straight geodesic on
( proper time, so is measured in metres along ); its coordinate velocity is the constant with ; and an ideal clock carried along it reads, between two coordinate times within that physical worldline's domain,
The maximal geodesic continuation is determined by alone; the free-fall postulate does not require the body's physical domain to be maximal.
(c) No tidal response. Every free-fall congruence of this model has vanishing relative acceleration: , since the curvature vanishes identically.
(d) Scope. The model is an idealized vacuum model of the framework, not a claim about the actual universe: no observation, apparatus, calibration or uncertainty is used, and no comparison with data is made. The flat model solves the field law with the chosen parameters ; other solutions of the same field law exist and are not excluded, and flat solutions with different global topology exist as well (see the scope remark of this page). The physical interpretation of coordinates, clocks and bodies remains the adopted one of the cited postulates.
Facts & Assumptions
Given: The adopted framework postulates in the direct-equation presentation, the flat model of The flat model spacetime: the Minkowski metric on R^4 and its inertial chart, the parameters and , and the vacuum prescription .
The model spacetime is a smooth time-oriented Lorentzian four-manifold without boundary, and the framework adopts the model's geometry and its matter content separately; a model that prescribes directly is admissible only if the prescription meets the consistency conditions imposed by the adopted field law (Adopted spacetime model and classical domain of the gravitational framework clauses (i) and (iv), Adopted matter-content assumptions: fields, equations, stress-energy and energy conditions clauses (ii)-(iii)).
The field law of the direct-equation presentation is with , and it is the model's adopted gravitational dynamics (Adopted Einstein field equation in the direct-equation presentation clause (i), SI unit and coordinate conventions of the classical gravitational framework clause (a), The Riemann curvature operator and the derived Ricci, scalar and Einstein tensors clause (c)).
An ideal freely falling massive test body of the model has as worldline a future timelike geodesic with , proper time an affine parameter, and on its actual domain the worldline is the restriction of the unique maximal geodesic determined by the release event and four-velocity; ideal clocks read the proper time of their worldline (Adopted clock, free-fall and light-ray assumptions of the classical gravitational framework clauses (i)-(ii), The free-fall worldline of an ideal test body is determined by its initial event and four-velocity, Timelike worldlines, proper time, length and four-velocity on a Lorentzian four-manifold, Proper time is well defined and reparametrization invariant; the four-velocity is its proper-time tangent).
In the inertial chart of the flat model the Christoffel symbols of the metric-selected connection vanish, the curvature tensor vanishes, , and the geodesics are the affinely parametrized straight lines: a geodesic has with constant , speed , maximal domain ; if and it is a future timelike worldline with four-velocity , , and coordinate velocity of norm (The flat model: vanishing connection and curvature, translation Killing fields and straight geodesics clauses (a)-(e), The flat model spacetime: the Minkowski metric on R^4 and its inertial chart clause (c), Metric compatibility, torsion freedom and the metric-selected connection class, Existence and uniqueness of the metric-selected connection of a nondegenerate metric, and its extension to tensor fields).
For the flat metric with and the field law holds identically, and with it fails; the consistency condition holds for (Consistency conditions of the adopted field law: conservation, trace, parameter variation and the energy conditions of a perfect fluid clause (d)).
If the curvature vanishes on an open set, every free-fall congruence with worldlines there satisfies (Free-fall congruences, tidal (curvature) relative acceleration and the flat comparison clause (c)).
A smooth free proper Lie-group action has a Hausdorff second-countable smooth quotient, and its projection is a surjective submersion (Left group actions, transitive actions, and faithful actions, Free and proper Lie-group actions, Free proper action quotient manifold). In equal dimensions its differential is invertible, so the projection is locally a diffeomorphism (The smooth inverse function theorem on manifolds). Covariant tensors pull back by applying the differential to their arguments (The pullback of a covariant tensor field).
Smooth parameter integrals over a fixed compact interval can be differentiated under compact domination; the fundamental theorem differentiates primitives and evaluates integrals of derivatives. Smooth mixed partials commute, and continuous real functions are bounded on compact sets (Differentiation under the integral sign, The first fundamental theorem: if is integrable on and continuous at , then ; in particular a continuous has as a primitive, The second fundamental theorem: if is differentiable on with and is integrable, then , The chain rule for total derivatives: , Clairaut--Schwarz theorem for continuous second partial derivatives, A continuous image of a compact space is compact; a continuous real-valued map on a nonempty compact space attains a maximum and a minimum; and a continuous bijection from a compact space to a Hausdorff space is a homeomorphism). The metric-selected Christoffel formula and its curvature contraction are those of Existence and uniqueness of the metric-selected connection of a nondegenerate metric, and its extension to tensor fields and Tensoriality of the curvature, its coordinate formula and its point-normal metric formula.
Proof
(The model and its field law.) By The flat model spacetime: the Minkowski metric on R^4 and its inertial chart clauses (a)-(c), is a smooth time-oriented Lorentzian four-manifold without boundary; by [A1] it satisfies the spacetime postulate, and is a smooth symmetric covariant -tensor field on the matter domain . By [L1], ; with and , holds identically, and trivially, so the prescription is admissible by [A1] and the field law holds by [A2]; this is also the flat vacuum solution of [L2]. This proves (a).
(Free fall and clock readings.) Let be as in (b), and write with , ; the normalization is possible by The flat model spacetime: the Minkowski metric on R^4 and its inertial chart clause (c). By [A3] the physical worldline is a restriction of the unique maximal future timelike geodesic through , with proper time as affine parameter. By [L1] this maximal mathematical geodesic is the straight line . With proper-time parametrization (the normalization of [L1]), this is ; the coordinate velocity is the constant with by [L1]. Finally, for two coordinate times in the physical domain, the ideal clock reads proper time by [A3], and from the parametrization along the line, ; since by [L1] clause (e), and hence . This proves (b).
(No tidal response.) The curvature vanishes identically by [L1], so by [L3] every free-fall congruence satisfies . This proves (c).
(Another flat vacuum model.) Fix a length . Let the discrete zero-dimensional Lie group act on by . Translations are smooth; the action is free since forces . For any compact set , both projections have bounded time coordinates, so its inverse image under has only finitely many integer components. Each component is closed in a compact projection of , hence compact; the inverse image is a finite union of compact sets. The action is therefore proper. By [F1], is a smooth four-manifold with a locally diffeomorphic projection . Define and by and ; these are well defined because translations preserve and . In each inverse chart of they are smooth with having constant components and . Thus is time-oriented and flat. With , , its Einstein tensor and stress divergence vanish, so it satisfies the same adopted vacuum field law and matter consistency condition.
(The quotient has different smooth global topology.) The translation-invariant covector descends to a smooth covector field on , with . Its coordinate components satisfy in every chart: in inverse charts they are constant, and the equality is preserved by coordinate changes by the chain rule and commuting mixed partials. The closed curve , , satisfies . If a diffeomorphism existed, write ; the same component symmetry holds for . Define . By [F2], . Hence . Its integral around would then be the endpoint difference of a single-valued smooth function and equal zero, contradicting . Thus is not diffeomorphic to , proving the different-topology assertion of (d).
(A non-flat vacuum solution.) On with length coordinates put and . The block has determinant and therefore one positive and one negative eigenvalue; the other two directions are positive. This is a smooth Lorentzian metric, time-oriented by , since . Its inverse has , , , and all other entries zero. Substitution into the Christoffel formula of [F2] gives only and for . The traces vanish, and the product terms in the Ricci contraction vanish: every nonzero symbol has a lower and either upper or two lower with transverse upper index, whereas every symbol with lower or upper is zero. Thus the only possible nonzero Ricci component is ; nevertheless . With , this gives another admissible vacuum solution of the same field law, now non-flat.
(Conclusion and status.) Steps 1.1-1.3 establish (a)-(c) for the stated Minkowski model; steps 1.4, 2.1 and 2.2 establish the comparison existence claims of (d). All use the adopted postulates and explicit mathematics, with no observation, apparatus or measured input. Neither these deductions nor the comparison constructions assert that any of the models is realized in nature.
Remarks
- One model among many. Nothing in the deduction selects the flat model uniquely: the field law admits non-flat solutions, and flat Lorentzian solutions with different global topology are not excluded by the local computations here. The model is used on this page as the flat comparison background of the weak-field bridge, not as a claim about the world.
- Presentations. The deduction uses the direct-equation presentation of the field law. In the action presentation the same model is described by the admitted scalar sector with constant , and , whose scalar stress tensor vanishes; the equivalence of the presentations on the stated domain is Stationarity of the adopted total action is equivalent to the Einstein equation with the framework's coupling, and no second adoption of the equation is implied.
Depends on
The flat model spacetime: the Minkowski metric on R^4 and its inertial chart
The flat model: vanishing connection and curvature, translation Killing fields and straight geodesics
Stationarity of the adopted total action is equivalent to the Einstein equation with the framework's coupling
Adopted spacetime model and classical domain of the gravitational framework
Adopted matter-content assumptions: fields, equations, stress-energy and energy conditions
Adopted Einstein field equation in the direct-equation presentation
Adopted clock, free-fall and light-ray assumptions of the classical gravitational framework
The free-fall worldline of an ideal test body is determined by its initial event and four-velocity
Consistency conditions of the adopted field law: conservation, trace, parameter variation and the energy conditions of a perfect fluid
Free-fall congruences, tidal (curvature) relative acceleration and the flat comparison
Stress-energy tensor field of a model
SI unit and coordinate conventions of the classical gravitational framework
Timelike worldlines, proper time, length and four-velocity on a Lorentzian four-manifold
Proper time is well defined and reparametrization invariant; the four-velocity is its proper-time tangent
The Riemann curvature operator and the derived Ricci, scalar and Einstein tensors
Smooth time-oriented Lorentzian four-manifolds: the geometric objects of the model
Metric compatibility, torsion freedom and the metric-selected connection class
Existence and uniqueness of the metric-selected connection of a nondegenerate metric, and its extension to tensor fields
Free proper action quotient manifold
Free and proper Lie-group actions
Left group actions, transitive actions, and faithful actions
The smooth inverse function theorem on manifolds
The pullback of a covariant tensor field
Differentiation under the integral sign
The first fundamental theorem: if is integrable on and continuous at , then ; in particular a continuous has as a primitive
The second fundamental theorem: if is differentiable on with and is integrable, then
The chain rule for total derivatives:
Clairaut--Schwarz theorem for continuous second partial derivatives
A continuous image of a compact space is compact; a continuous real-valued map on a nonempty compact space attains a maximum and a minimum; and a continuous bijection from a compact space to a Hausdorff space is a homeomorphism
Tensoriality of the curvature, its coordinate formula and its point-normal metric formula
Dependency tree · 2 levels
Sources
- S. M. Carroll, Lecture Notes on General Relativity, arXiv:gr-qc/9712019v1 (1997), Ch. 1: Minkowski spacetime, inertial coordinates and the free motion of test particles; Ch. 4: the vacuum field equations with Lambda=0, printed pp. 6-20 (PDF pp. 13-27) and pp. 113-120 (PDF pp. 120-127)
- D. Tong, General Relativity (Cambridge Part III Mathematical Tripos, Michaelmas 2019), section 1.2: the Minkowski metric, inertial worldlines and proper time; section 4.1: the vacuum equations G=0 and the flat solution, printed pp. 12-29 (PDF pp. 19-36) and pp. 140-144 (PDF pp. 147-151)
- H. S. Reall, Part III General Relativity (Cambridge, October 12, 2022 revision), section 4.2: zero curvature of Minkowski space and local flatness, printed p. 42 (PDF p. 43); section 6.4: the adopted field law and vacuum equation Ric=0, (6.32)-(6.33), printed p. 67 (PDF p. 68); the comparison models and topology obstruction are verified locally